二维内部重力波束不稳定性。线性理论与亚临界不稳定性

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2021-08-04 DOI:10.1080/03091929.2021.1943379
U. Harlander, M. Kurgansky
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引用次数: 1

摘要

内部重力波的不稳定性一直是地球物理流体动力学研究的热点,因为内部重力波的破裂与大尺度气流交换能量和动量,从而支持大尺度环流。在本研究中,使用低阶IGW梁模型来描述线性和所谓的非模态瞬态不稳定性。第一部分采用Galerkin方法研究了由两个相同频率、不同量级平行波矢的有限振幅平面单色igw组成的波束的线性正态失稳问题。得出的结论是,波束在线性上比其组成的平面波更不稳定。不稳定程度随组成波在波数空间的分离而增大,即随波束在物理空间的集中而增大。波束越窄,它的线性不稳定性就越强。反过来,瞬态不稳定通常发生在线性稳定的流动中,或者在控制系统矩阵是非正态的情况下,在线性不稳定发生之前(亚临界不稳定)。在论文的第二部分,首先通过计算方法如亨里希数、伪谱和矩阵的值域来检验波束模型的线性系统矩阵的非正态性。然后,研究了最优增长初始条件随机摄动时的瞬态增长的鲁棒性。结论是,对于完全随机化,特别是浅波光束在进入湍流背景场时可以表现出亚临界增长。这种不断增长并最终破裂的波束可能会在现有的背景湍流中增加湍流,这种背景湍流源于其他不稳定的来源。然而,波束扰动的瞬态增长的鲁棒性在很大程度上取决于初始条件、波束角和扰动波长的随机化强度。
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Two-dimensional internal gravity wave beam instability. Linear theory and subcritical instability
The instability of propagating internal gravity waves (IGWs) is of long-standing interest in geophysical fluid dynamics since breaking IGWs exchange energy and momentum with the large-scale flow and hence they support the large-scale circulation. In this study a low-order IGW beam model is used to delineate both linear and so called non-modal transient instability. In the first part of the study, linear normal mode instability of a wave beam consisting of two finite-amplitude plane monochromatic IGWs with the same frequency and parallel wave vectors of different magnitude is investigated using the Galerkin method. It is concluded that the wave beam is linearly more unstable than its constituent plane waves, taken separately. The degree of instability increases with the separation of the constituent waves in the wave number space, that is, with the wave beam concentration in the physical space. The narrower a wave beam is, the more linearly unstable it is. In its turn, transient instability typically occurs for linearly stable flows or before linear instability can set in (subcritical instability) if the governing system matrix is non-normal. In the second part of the paper, first the non-normality of the linear system matrix of the wave beam model is examined by computing measures like the Henrici number, the pseudospectrum, and the range of the matrix. Subsequently, the robustness of the transient growth is studied when the initial condition for optimal growth is randomly perturbed. It is concluded that for full randomisation, in particular, shallow wave beams can show subcritical growth when entering a turbulent background field. Such growing and eventually breaking wave beams might add turbulence to existing background turbulence that originates from other sources of instability. However, the robustness of transient growth for wave beam perturbations depends strongly on the strength of randomisation of the initial conditions, the beam angle and the perturbation wavelength.
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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